Previously, astronomers had been under the impression that the heavy elements—gold, platinum, lead, uranium, etc.—came from supernova explosions. But now, scientists have announced a new theory for these highly valuable elements, this one involving two ultra-dense neutron stars and one spectacularly violent, grossly expensive collision.
We Are All Made of Stars
Essentially, we’re all here to today because some star somewhere in space exploded once upon a time. Down in the interior of stars, the high pressure and heat cooks up elements like carbon and oxygen atoms (the stuff we’re made of). So when it inevitably comes time for that star to die, that explosion shoots out all of the ingredients for life as we know it.
This explanation didn’t, however, quite manage to explain where the more dense elements got their start. Because while the majority of light elements come with a fairly simple recipe, a heavier one like gold requires 79 protons, 79 electrons, and 118 neutrons—that’s a hell of lot of ingredients. Which is why it takes these absurdly dense neutron stars, which come packing way more atomic supplies, to give us all those beautiful, heavy, glittering goods.
What’s a Neutron Star?
When a massive star enters Type II, Type Ib, or Type Ic supernova—or in other words, when its core is essentially crushed by the force of its own gravity—there are two potential outcomes. It can either turn into a black hole or emerge from its supernova cocoon as a neutron star. To the get the latter, you’d need to start with a star about 4 to 8 times the size of our sun. Once the star burns off enough nuclear fuel to the point that the core can no longer support itself, gravity finally wins and collapses the core with enough force to cause protons and electrons to assimilate. Which creates neutrons. Which, as you may have already guessed, is where neutron stars get their name.
To get an idea of just how dense a neutron star is, a mere teaspoon of the stuff would weigh about 10 billion tons. (Of course, if you actually did extract a teaspoon of neutronium goo, you’d lose all that wonderful gravitational force holding everything together, and the whole thing would immediately explode into a giant mass of neutrons about the size of a planet that would then break down to its individual proton and electron parts. To put it bluntly, you, dear reader, would die. But that’s neither here nor there.)
When Two Neutron Stars Love Each Other Very Much…
So under most circumstances, these insanely dense dead stars will float around the universe doing no one any harm. But in binary star systems, the two are destined to collide. And this is what NASA‘s Swift space telescope observed during an all-sky survey on June 3.
After seeing a flash of light called a short gamma-ray burst (GRB) far, far way in the constellation Leo, astronomers were quickly able to deduce (with the help of a few theoretical models) that what they were seeing was the radioactive afterglow from a gargantuan mass of heavy metals created in the wake of a neutron star collision. Previously, scientists had only been able to hypothesize that GRBs were the result of two colliding neutron stars, but now we have actual proof.
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